Table 1.
Non-magnetic CVs found in the RBS.
RBS# | Name | D̃ (pc) |
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fX (erg cm−2 s−1) | p (mas) | Δp (mas) | log LX (s−1) | D (pc) | Dmax (pc) | Vgen (pc3) |
---|---|---|---|---|---|---|---|---|---|---|
2 | EF Tuc | 500: | 32.0 | 3.38E–12 | 0.720 | 0.023 | 32.9 | 1335 | 1462 | 2.09E+08 |
22 | WW Cet | 100 | 31.0 | 9.16E–12 | 4.588 | 0.047 | 31.7 | 216 | 389 | 3.28E+07 |
280 | TT ARI | 135 | 31.1 | 5.96E–12 | 3.884 | 0.070 | 31.7 | 256 | 372 | 4.20E+07 |
288 | WX HYI | 265 | 31.6 | 6.26E–12 | 4.273 | 0.029 | 31.6 | 232 | 346 | 3.21E+07 |
372 | IQ Eri | 130 | 30.8 | 3.76E–12 | 5.186 | 0.167 | 31.2 | 192 | 222 | 1.11E+07 |
490 | 33 | 29.6 | 3.36E–12 | 3.098 | 0.126 | 31.6 | 320 | 349 | 3.51E+07 | |
512 | VW Hyi | 65 | 30.9 | 1.59E–11 | 18.531 | 0.022 | 30.7 | 54 | 128 | 3.26E+06 |
664 | TW Pic | – | – | 3.13E–12 | 2.284 | 0.022 | 31.8 | 432 | 455 | 7.99E+07 |
694 | SU UMa | 280 | 32.1 | 1.41E–11 | 4.535 | 0.029 | 31.9 | 219 | 490 | 9.25E+07 |
710 | SW UMa | 140 | 30.9 | 3.81E–12 | 6.148 | 0.080 | 31.1 | 162 | 188 | 9.09E+06 |
(713 | EI UMa) | – | – | |||||||
728 | BZ UMa | 110 | 30.9 | 6.12E–12 | 6.557 | 0.064 | 31.2 | 152 | 224 | 1.39E+07 |
1008 | T Leo | 100 | 31.1 | 9.88E–12 | 7.814 | 0.069 | 31.3 | 128 | 240 | 1.33E+07 |
1411 | RHS40 | 460 | 32.0 | 3.47E–12 | 2.919 | 0.671 | 31.7 | 367 | 407 | 3.72E+07 |
1900 | TY PsA | 300: | 31.7 | 4.68E–12 | 5.431 | 0.065 | 31.3 | 183 | 236 | 1.26E+07 |
1955 | V405 Peg | 30 | 29.5 | 3.05E–12 | 5.784 | 0.062 | 31.0 | 172 | 179 | 8.06E+06 |
1969 | CC Scl | 165 | 31.1 | 4.23E–12 | 4.904 | 0.148 | 31.3 | 203 | 249 | 1.37E+07 |
Notes. #713 is no longer considered non-magnetic, whereas #664 was previously classified as an IP. The luminosity is given in the ROSAT spectral band 0.1–2.4 keV. Distances and luminosities from Schwope et al. (2002) are listed in columns with tildes, all other values are from this work. Vgen was computed for a scale height of 200 pc.
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